VizieR Online Data Catalog: PTF12os and iPTF13bvn spectra and light curves (Fremling+, 2016)

(1)

2016

Publication Year

2020-07-23T13:40:34Z

Acceptance in OA@INAF

VizieR Online Data Catalog: PTF12os and iPTF13bvn spectra and light curves

(Fremling+, 2016)

Title

Fremling, C.; Sollerman, J.; Taddia, F.; Ergon, M.; Fraser, M.; et al.

Authors

10.26093/cds/vizier.35930068

DOI

http://hdl.handle.net/20.500.12386/26596

Handle

VizieR Online Data Catalog

Journal

(2)

7/1/2020 J/A+A/593/A68

https://cdsarc.unistra.fr/viz-bin/ReadMe/J/A+A/593/A68?format=html&tex=true 1/2

J/A+A/593/A68 PTF12os and iPTF13bvn spectra and light curves (Fremling+, 2016) PTF12os and iPTF13bvn:

Two stripped-envelope supernovae from low-mass progenitors in NGC 5806. Fremling C., Sollerman J., Taddia F., Ergon M., Fraser M.,

Karamehmetoglu E., Valenti S., Jerkstrand A., Arcavi I., Bufano F., Elias Rosa N., Filippenko A.V., Fox D., Gal-Yam A., Howell D.A.,

Kotak R., Mazzali P., Milisavljevic D., Nugent P.E., Nyholm A., Pian E., Smartt S.

<Astron. Astrophys. 593, A68 (2016)>

=2016A&A...593A..68F (SIMBAD/NED BibCode)

ADC_Keywords: Supernovae ; Photometry, UBVRI ; Photometry, SDSS ; Spectroscopy Keywords: supernovae: general - supernovae: individual: PTF12os -

galaxies: individual: NGC 5806 - techniques: image processing - supernovae: individual: iPTF13bvn

Abstract:

We investigate two stripped-envelope supernovae (SNe) discovered in the nearby galaxy NGC 5806 by the (i)PTF. We classify PTF12os as a Type IIb SN based on our spectral sequence; iPTF13bvn has previously been classified as Type Ib. Our main objective is to constrain the explosion parameters of iPTF12os and iPTF13bvn, and to put constraints on the SN progenitors, using our comprehensive photometric and

spectroscopic datasets. Description:

Photometric and spectroscopic datasets of PTF12os and iPTF13bvn. Our dataset on PTF12os spans from approximately 8.5 days to 215 days past the SN explosion and it contains optical photometry and spectra. Our data on iPTF13bvn spans from approximately 0.6 to 380 days. The dataset on iPTF13bvn contains optical photometry and optical/infrared spectroscopy. Objects: --- RA (2000) DE Designation(s) --- 14 59 59.12 +01 53 24.4 PTF12os = SN 2012P 15 00 00.15 +01 52 53.2 iPTF13bvn = iPTF 13bvn --- File Summary:

FileName Lrecl Records Explanations

ReadMe 80 . This file

ph12os.dat 33 264 Bgriz photometry of PTF12os ph13bvn.dat 33 461 UBVRIgriz photometry of iPTF13bvn sw12os.dat 43 6 Swift/UVOT photometry of PTF12os sw13bvn.dat 43 9 Swift/UVOT photometry of iPTF13bvn sp12os.dat 52 19 Spectroscopic observations of PTF12os sp13bvn.dat 52 32 Spectroscopic observations of iPTF13bvn sp/* 19 51 Individual spectra

Byte-by-byte Description of file: ph12os.dat ph13bvn.dat

Bytes Format Units Label Explanations

1- 11 F11.3 d JD Julian date of observation 13- 18 F6.3 mag mag Apparent magnitude (1)

20- 24 F5.3 mag e_mag Uncertainty (1 sigma) of apparent magnitude 26 A1 --- Filter [UBVRIgriz] Photometric filter

28- 33 A6 --- Tel Telescope (G2)

Note (1): Johnson-Cousins filter magnitudes are given in the Vega system. Sloan filter magnitudes are in the AB system.

Byte-by-byte Description of file: sw12os.dat sw13bvn.dat

1- 10 F10.2 d JD Julian date of observation

12- 16 F5.2 mag Umag ?=99.99 Apparent U-band AB magnitude 18- 21 F4.2 mag e_Umag ?=9.99 Uncertainty (1 sigma) of U magnitude 23- 27 F5.2 mag UVW1mag ?=99.99 Apparent UVW1-band AB magnitude 29- 32 F4.2 mag e_UVW1mag ?=9.99 Uncertainty (1 sigma) of UVW1 magnitude

Portal

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7/1/2020 J/A+A/593/A68

https://cdsarc.unistra.fr/viz-bin/ReadMe/J/A+A/593/A68?format=html&tex=true 2/2

• Contact © Université de Strasbourg/CNRS 34- 38 F5.2 mag UVM2mag ?=99.99 Apparent UVM2-band AB magnitude

40- 43 F4.2 mag e_UVM2mag ?=9.99 Uncertainty (1 sigma) of UVM2 magnitude

Byte-by-byte Description of file: sp12os.dat sp13bvn.dat

1- 10 F10.2 d JD Julian date of observation 12- 17 F6.2 d Phase Time since supernova explosion 19- 37 A19 --- TelInst Name of telescope/instrument (G1) 39- 52 A14 --- FileName Name of spectrum file in subdirectory sp

Byte-by-byte Description of file: sp/*

1- 8 F8.2 0.1nm lambda Wavelength 10- 19 E10.4 --- Flux Observed flux (1)

Note (1): The spectra are uncalibrated and fluxes are given in arbitrary units.

Global Notes:

Note (G1): the telescopes used for the spectroscopy are as follows: CA/CAFOS = Calar Alto 2.2m Telscope

FTS/FLOYDS = Faulkes Telescope North FTS/FLOYDS = Faulkes Telescope South NOT/ALFOSC = Nordic Optical Telescope

P200/DBSP = Palomar 200-inch (5.1-meter) Hale Telescope TNG/LRS = Telescopie Nazionale Galileo

WHT/ISIS = William Herschel Telescope Magellan_Baade/FIRE = The Magellan Telescopes (6.5m) IRTF/SpeX = NASA Infrared Telescope Facility

KECK1/LRIS = The Keck 1 Telescope at W. M. Keck Observatory KECK2/DEIMOS = The Keck 2 Telescope at W. M. Keck Observatory VLT/FORS2 = The Very Large Telescope

APO/DIS = Apache Point ARC 3.5m Telescope SALT/Spectrograph = The Southern African Large Telescope ASIAGO/AFOSC = The 182cm Copernico telescope

KPNO/RCSpec = Kitt Peak National Observatory's Mayall 4-m Telescope LICK/KAST = The Lick Observatory Shane 3-m Telescope

GTC/OSIRIS = Gran Telescopio Canarias

NTT/EFOSC = The 3.58-meter New Technology Telescope

GEMINI_N/GMOS = The Frederick C. Gillett Gemini North Telescope Note (G2): the telescopes used for the photometry are as follows: P48 = Palomar 48-inch Samuel Oschin Telescope

P60 = Palomar 60-inch (1.5-meter) Telescope P200 = Palomar 200-inch (5.1-meter) Hale Telescope LCOGT = Las Cumbres Observatory Global Telescope Network NOT = Nordic Optical Telescope

NTT = The 3.58-meter New Technology Telescope LT = The Liverpool Telescope

GTC = Gran Telescopio Canarias

Acknowledgements:

Christoffer Fremling, christoffer.fremling(at)astro.su.se

(End) Christoffer Fremling [Stockholm Univ.], Patricia Vannier [CDS] 07-Jul-2016

The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load ﬁles into arrays or line by line